An ultraluminous X-ray source powered by an accreting neutron star

M. Bachetti, F.A. Harrison, D.J. Walton, B.W. Grefenstette, D. Chakrabarty, F. Fürst, D. Barret, A. Beloborodov, S.E. Boggs, F.E. Christensen, W.W. Craig, A.C. Fabian, C.J. Hailey, A. Hornschemeier, V. Kaspi, S.R. Kulkarni, Thomas Maccarone, J.M. Miller, V. Rana, D. SternS.P. Tendulkar, J. Tomsick, N.A. Webb, W.W. Zhang

Research output: Contribution to journalArticle

Original languageEnglish
Pages (from-to)202-204
JournalNature
StatePublished - Oct 2014

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Bachetti, M., Harrison, F. A., Walton, D. J., Grefenstette, B. W., Chakrabarty, D., Fürst, F., Barret, D., Beloborodov, A., Boggs, S. E., Christensen, F. E., Craig, W. W., Fabian, A. C., Hailey, C. J., Hornschemeier, A., Kaspi, V., Kulkarni, S. R., Maccarone, T., Miller, J. M., Rana, V., ... Zhang, W. W. (2014). An ultraluminous X-ray source powered by an accreting neutron star. Nature, 202-204.